Black Holes as High-Density Space Quanta: Singularity Avoidance and Modified Evaporation in the Time Field Model

We redefine black holes in the Time Field Model (TFM) as massive space quanta—a wave-based solution that removes central singularities and modifies evaporation. By treating black holes as high-density condensates of T±-field quanta, we derive a Schwarzschild-like metric with a Planck-core cutoff, link the horizon radius and entropy to prior TFM parameters (λβ²), and propose a wave-decoherence evaporation rate. Our calculations predict observable deviations of 1–10% in ringdown frequencies (LIGO/Virgo/LISA) at signal-to-noise ratio (SNR) ≳ 30, and up to 1% changes in black hole shadow sizes (EHT). We contrast TFM with loop-quantum black hole and fuzzball proposals, unifying cosmic and BH scales (Paper #13) via wave lumps. HPC simulations confirm Planck-core stability under wave-lump collapse, implemented via a modified Einstein Toolkit. Finally, we propose a time-wave accretion model for supermassive black hole (SMBH) formation at z > 7, testable in joint HPC–observational campaigns.